γ-ray strength function and pygmy resonance in rare earth nuclei
The γ-ray strength function for γ energies in the 1–7 MeV region has been measured for 161,162Dy and 171,172Yb using the (3He,αγ) reaction. Various models are tested against the observed γ-ray strength functions. The best description is based on the Kadmenskiĭ, Markushev, and Furman E1 model with co...
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E-Artikel |
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2001 |
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Online-Ressource 7 |
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APS Digital Backfile Archive 1893-2003 |
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| Übergeordnetes Werk: |
Enthalten in: Physical review / C - Woodbury, NY : Inst., 1970, 63(2001), 4 |
| Übergeordnetes Werk: |
volume:63 ; year:2001 ; number:4 ; extent:7 |
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| 520 | |a The γ-ray strength function for γ energies in the 1–7 MeV region has been measured for 161,162Dy and 171,172Yb using the (3He,αγ) reaction. Various models are tested against the observed γ-ray strength functions. The best description is based on the Kadmenskiĭ, Markushev, and Furman E1 model with constant temperature and the Lorentzian M1 model. A γ-ray bump observed at Eγ∼3 MeV is interpreted as the so-called pygmy resonance, which has also been observed previously in (n,γ) experiments. The parameters for this resonance have been determined and compared to the available systematics. | ||
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(DE-627)NLEJ249700026 (DE-601)aps:a0a95c52d18fae4ddd9757f2bb17933de8169644 DE-627 ger DE-627 rakwb γ-ray strength function and pygmy resonance in rare earth nuclei 2001 Online-Ressource 7 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The γ-ray strength function for γ energies in the 1–7 MeV region has been measured for 161,162Dy and 171,172Yb using the (3He,αγ) reaction. Various models are tested against the observed γ-ray strength functions. The best description is based on the Kadmenskiĭ, Markushev, and Furman E1 model with constant temperature and the Lorentzian M1 model. A γ-ray bump observed at Eγ∼3 MeV is interpreted as the so-called pygmy resonance, which has also been observed previously in (n,γ) experiments. The parameters for this resonance have been determined and compared to the available systematics. APS Digital Backfile Archive 1893-2003 Voinov, A. oth Enthalten in Physical review / C Woodbury, NY : Inst., 1970 63(2001), 4 Online-Ressource (DE-627)NLEJ24823787X (DE-600)1461161-2 1089-490X nnns volume:63 year:2001 number:4 extent:7 https://www.tib.eu/de/suchen/id/aps%3Aa0a95c52d18fae4ddd9757f2bb17933de8169644 Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 63 2001 4 7 |
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(DE-627)NLEJ249700026 (DE-601)aps:a0a95c52d18fae4ddd9757f2bb17933de8169644 DE-627 ger DE-627 rakwb γ-ray strength function and pygmy resonance in rare earth nuclei 2001 Online-Ressource 7 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The γ-ray strength function for γ energies in the 1–7 MeV region has been measured for 161,162Dy and 171,172Yb using the (3He,αγ) reaction. Various models are tested against the observed γ-ray strength functions. The best description is based on the Kadmenskiĭ, Markushev, and Furman E1 model with constant temperature and the Lorentzian M1 model. A γ-ray bump observed at Eγ∼3 MeV is interpreted as the so-called pygmy resonance, which has also been observed previously in (n,γ) experiments. The parameters for this resonance have been determined and compared to the available systematics. APS Digital Backfile Archive 1893-2003 Voinov, A. oth Enthalten in Physical review / C Woodbury, NY : Inst., 1970 63(2001), 4 Online-Ressource (DE-627)NLEJ24823787X (DE-600)1461161-2 1089-490X nnns volume:63 year:2001 number:4 extent:7 https://www.tib.eu/de/suchen/id/aps%3Aa0a95c52d18fae4ddd9757f2bb17933de8169644 Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 63 2001 4 7 |
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(DE-627)NLEJ249700026 (DE-601)aps:a0a95c52d18fae4ddd9757f2bb17933de8169644 DE-627 ger DE-627 rakwb γ-ray strength function and pygmy resonance in rare earth nuclei 2001 Online-Ressource 7 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The γ-ray strength function for γ energies in the 1–7 MeV region has been measured for 161,162Dy and 171,172Yb using the (3He,αγ) reaction. Various models are tested against the observed γ-ray strength functions. The best description is based on the Kadmenskiĭ, Markushev, and Furman E1 model with constant temperature and the Lorentzian M1 model. A γ-ray bump observed at Eγ∼3 MeV is interpreted as the so-called pygmy resonance, which has also been observed previously in (n,γ) experiments. The parameters for this resonance have been determined and compared to the available systematics. APS Digital Backfile Archive 1893-2003 Voinov, A. oth Enthalten in Physical review / C Woodbury, NY : Inst., 1970 63(2001), 4 Online-Ressource (DE-627)NLEJ24823787X (DE-600)1461161-2 1089-490X nnns volume:63 year:2001 number:4 extent:7 https://www.tib.eu/de/suchen/id/aps%3Aa0a95c52d18fae4ddd9757f2bb17933de8169644 Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 63 2001 4 7 |
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(DE-627)NLEJ249700026 (DE-601)aps:a0a95c52d18fae4ddd9757f2bb17933de8169644 DE-627 ger DE-627 rakwb γ-ray strength function and pygmy resonance in rare earth nuclei 2001 Online-Ressource 7 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The γ-ray strength function for γ energies in the 1–7 MeV region has been measured for 161,162Dy and 171,172Yb using the (3He,αγ) reaction. Various models are tested against the observed γ-ray strength functions. The best description is based on the Kadmenskiĭ, Markushev, and Furman E1 model with constant temperature and the Lorentzian M1 model. A γ-ray bump observed at Eγ∼3 MeV is interpreted as the so-called pygmy resonance, which has also been observed previously in (n,γ) experiments. The parameters for this resonance have been determined and compared to the available systematics. APS Digital Backfile Archive 1893-2003 Voinov, A. oth Enthalten in Physical review / C Woodbury, NY : Inst., 1970 63(2001), 4 Online-Ressource (DE-627)NLEJ24823787X (DE-600)1461161-2 1089-490X nnns volume:63 year:2001 number:4 extent:7 https://www.tib.eu/de/suchen/id/aps%3Aa0a95c52d18fae4ddd9757f2bb17933de8169644 Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 63 2001 4 7 |
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(DE-627)NLEJ249700026 (DE-601)aps:a0a95c52d18fae4ddd9757f2bb17933de8169644 DE-627 ger DE-627 rakwb γ-ray strength function and pygmy resonance in rare earth nuclei 2001 Online-Ressource 7 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The γ-ray strength function for γ energies in the 1–7 MeV region has been measured for 161,162Dy and 171,172Yb using the (3He,αγ) reaction. Various models are tested against the observed γ-ray strength functions. The best description is based on the Kadmenskiĭ, Markushev, and Furman E1 model with constant temperature and the Lorentzian M1 model. A γ-ray bump observed at Eγ∼3 MeV is interpreted as the so-called pygmy resonance, which has also been observed previously in (n,γ) experiments. The parameters for this resonance have been determined and compared to the available systematics. APS Digital Backfile Archive 1893-2003 Voinov, A. oth Enthalten in Physical review / C Woodbury, NY : Inst., 1970 63(2001), 4 Online-Ressource (DE-627)NLEJ24823787X (DE-600)1461161-2 1089-490X nnns volume:63 year:2001 number:4 extent:7 https://www.tib.eu/de/suchen/id/aps%3Aa0a95c52d18fae4ddd9757f2bb17933de8169644 Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 63 2001 4 7 |
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The γ-ray strength function for γ energies in the 1–7 MeV region has been measured for 161,162Dy and 171,172Yb using the (3He,αγ) reaction. Various models are tested against the observed γ-ray strength functions. The best description is based on the Kadmenskiĭ, Markushev, and Furman E1 model with constant temperature and the Lorentzian M1 model. A γ-ray bump observed at Eγ∼3 MeV is interpreted as the so-called pygmy resonance, which has also been observed previously in (n,γ) experiments. The parameters for this resonance have been determined and compared to the available systematics. |
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The γ-ray strength function for γ energies in the 1–7 MeV region has been measured for 161,162Dy and 171,172Yb using the (3He,αγ) reaction. Various models are tested against the observed γ-ray strength functions. The best description is based on the Kadmenskiĭ, Markushev, and Furman E1 model with constant temperature and the Lorentzian M1 model. A γ-ray bump observed at Eγ∼3 MeV is interpreted as the so-called pygmy resonance, which has also been observed previously in (n,γ) experiments. The parameters for this resonance have been determined and compared to the available systematics. |
| abstract_unstemmed |
The γ-ray strength function for γ energies in the 1–7 MeV region has been measured for 161,162Dy and 171,172Yb using the (3He,αγ) reaction. Various models are tested against the observed γ-ray strength functions. The best description is based on the Kadmenskiĭ, Markushev, and Furman E1 model with constant temperature and the Lorentzian M1 model. A γ-ray bump observed at Eγ∼3 MeV is interpreted as the so-called pygmy resonance, which has also been observed previously in (n,γ) experiments. The parameters for this resonance have been determined and compared to the available systematics. |
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